README web version of /home/usg/OPS/MTS/readme_xml/readme_75010700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Hello,
The findercharts are all made with 2MASS and have the same size: 70" by 70". The
source is always located in the centre of the field. Unfortunately, the spatial
resolution is very low.
This programme includes objects of different multiplicities. For most of them, the
slit should be aligned such that 2 objects fall on the slit simultaneously. I have
arranged that by changing the rotator on the sky and the chopping angle (in parallel
mode).
On each OB, I also list the separation and PA of the different objects.
It would be good that, if an object is observed at e.g. 8.8um it will also be observed
at 11.4um, so that I can cover the whole range. Just a part of that region is pretty
useless to me. Unfortunately, I can't combine them in one OB as they would be too
long
in that case.
Please contact me if something remains unclear. Many thanks!
Gwendolyn Meeus
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
If the provided finding chart is at a different wavelength than the observations,
did you clearly describe in the README file how to identify the target?
Did you specify a guide star brighter than V=12mag within a field of
r=5arcmin around the science target?
Last creation of page: Tue Oct 6 15:40:06 2009
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